"The more than 70 terabytes we collected during the third epoch of this survey, SDSS-III, contain information on nearly half-a-billion stars and galaxies, including three-dimensional cosmic structures that formed billions of years before the sun began to shine," Schneider said. "This data release will undoubtedly form the basis for many future scientific investigations." Schneider is the SDSS-III survey coordinator and the project's scientific publication coordinator.
Niel Brandt, Penn State's Verne M. Willaman Professor of Astronomy and Astrophysics, is the SDSS-III leader of a number of projects investigating the properties of quasars, which are supermassive black holes that are devouring enormous amounts of matter, releasing amazing amounts energy in the process. "SDSS-III consists of four independent surveys," he said. "The fields range from searches for planets around nearby stars, to the chemical and dynamical evolution of our galaxy, to the large-scale structure of our universe."
After a decade of design and construction, the SDSS team began mapping the cosmos in 1998, using the dedicated 2.5-meter Sloan Foundation Telescope at Apache Point Observatory in New Mexico. Each phase of the project has used this telescope, which is equipped with a succession of powerful instruments, for a distinct set of astronomical surveys. SDSS-III started observations in July 2008 and completed its six-year, $45 million program in June 2014. The SDSS-III Collaboration includes 51 member institutions and 1,000 scientists from around the world.
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